木星 ALPO-Japan Latest
Jupiter Image 2020/10/02(UT)
伊藤了史,青木和夫,高尾幸弘,永長英夫,安達 誠,菅野清一
Christopher Go,Anthony Wesley,Ecleido Sousa Azevedo,Trevor Barry,Manos Kardasis,Strikis Iakovos
Christopher Go,S.Ito,K.Aoki,Y.Takao,Anthony.W,H.Einaga,M.Adachi,S.Kanno,E.S.Azevedo,T.Barry,Kardasis,S.Iakovos
Transparency was poor today due to clouds. Seeing was below average.
These images show the NTB Outbreak #1. It is now closing in on the tail where it will dissipate.
This might happen in the next 2 days. The NEB is dark and wide and has some complex rifiting.
[Christopher Go : Cebu Philippines]
≪愛知県 春日井市 伊藤了史≫[Satoshi Ito. Kasugai City,Aichi,Japan]
夕刻までは快晴でしたが、その後どんどん雲が増え
薄雲越しに１ショット撮ったところで全天雲に覆われてしまいました
[青木和夫:東京都世田谷区][Kazuo Aoki:Tokyo Japan]
最初に始めたIR撮影中にシーイングがさらに悪化、また雲も来てまともなカラー撮影はできませんでした。
<<北海道札幌市 高尾幸弘>>[Yukihiro Takao.Sapporo-city,Hokkaido,Japan]
Hi all,here's an RGB image of Jupiter from last night in a short spell
of good seeing. The head of NTB storm #1 is rising at top left,and the
NEB/NTB looks very disrupted across this hemisphere from the passage of
multiple NTB storms over the last few weeks.
[Anthony Wesley,Murrumbateman Australia]
≪アンソニ オーストラリア≫
[Hideo Einaga Kasai-City Hyogo-Prefecture Japan]
≪兵庫県 加西 永長英夫≫
ダイニック・アストロパーク・天究館にインストラクターでいったついでに
６０ｃｍで観測を試みた。シーイングの悪いことは分かっていたが、色を見たくて
少し期待していた。しかし、それを打ち破るほどの悪シーイングで、がっくりでした。
--------------------------------------------------------------
≪滋賀県 大津市 安達 誠≫[Makoto Adachi:Siga Japan]
10月に入って最初の撮像でしたがシーイングが良くなく、カラ-画像以外はボツにしました。
ボケボケの画像ですが、なんとか「NTBs jetstｒeam outbreak」＃2の後半部分は、確認出来ます
≪山形県上山市 菅野清一≫[Seiichi Kanno:Yamagata Japan]
[Ecleido Sousa Azevedo : Areado/MG,Brasil]
Imaged Jupiter October 2nd in mostly good seeing.
The head of outbreak #1 is seen toward the end of this session coming over the F limb.
It is preceded by the quite incredible linear structure still visible from the other outbreaks.
These data resolve a plethora of tiny compact dark spots within the NPR,two bright ovals are well resolved on the Southern edge of the NPR near the CM.
There extremely delicate structure within the NEB is well resolved from limb to limb.
A highlight of these data are the quite black features which seem associated with festoons in the EZ;
although these have been prominent at least since February they have become even darker,thinner and just so delicate.
The dark feature near the CM in these IR,R,G & B data is accompanied by two very compact bright spots v-close together just under the F end on the Southern edge of the NEB.
A prominent small bright oval is well seen on the Northern edge of the SPR.
Have also produced a multi-spectral animation of
IR,R,G,B,CH4,IR which provides quite interesting context regarding how the detail in these data is resolved at these various wavelengths.
>
[Trevor Barry:Broken Hill:Australia]
[Manos Kardasis,Glyfada-Athens;Greece]
《カーダシス マノス:ギリシャ アテネ》
[Strikis Iakovos : Athens,Greece]
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